Five New Multicomponent Planetary Systems

By S. Vogt, R. P. Butler, G. Marcy, Debra A. Fischer, G. Henry, Gregory Laughlin, Jason T. Wright, J. Johnson. 2005

186 citations recorded by the source corpus.

View Paper: https://www.semanticscholar.org/paper/d65486391d9109ab39f1d91403593462e9fa7b08

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In Astronomy and Astrophysics

Citations in the corpus

The planet search programme at the ESO CES and HARPS - IV. The search for Jupiter analogues around solar-like stars (2012, background): “5, 2 The planet was confirmed by Vogt et al. (2005) who revised the semi-major axis to 3.9 AU and discovered a second inner planet (17.1 d, 0.057MJup).”
Systemic: A Testbed for Characterizing the Detection of Extrasolar Planets. I. The Systemic Console Package (2009, methodology): “Therefore, while we have strengthened the case for models of HD128311 that only librate in θ1, a secure determination of the libration amplitude of ∆̟ might be obtained either by a transit monitoring campaign or yet additional RV measurements.”
Properties of planets in binary systems - The role of binary separation (2006, background): “Vogt et al. (2005) also report non detection of stellar companions at separations larger than 0.1 arcsec.”
THE CALIFORNIA PLANET SURVEY. I. FOUR NEW GIANT EXOPLANETS (2010, unknown): “The other such planets—55Cncd (Fischer et al. 2008), HD217107c (Vogt et al. 2005; Wright et al. 2009) and HD187123c (Wright et al. 2007, 2009)—are all in multi-planet systems.”
Mass-Radius Relationships for Solid Exoplanets (2007, unknown): “…fourteen exoplanets with Mp sin i < 21M⊕ (Butler et al. 2004; McArthur et al. 2004; Santos et al. 2004; Rivera et al. 2005; Bonfils et al. 2005; Vogt et al. 2005; Lovis et al. 2006; Udry et al. 2006; Bonfils et al. 2007; Melo et al. 2007), including one with Mp = 7.5M⊕ (Rivera et al. 2005)…”
EFFICIENT FITTING OF MULTIPLANET KEPLERIAN MODELS TO RADIAL VELOCITY AND ASTROMETRY DATA (2009, methodology): “To quantify this improvement, we tested two cases with published RV data, the 2-planet system HD 217107 (Vogt et al. 2005) and the 5-planet system 55 Cnc (Fischer et al. 2008) (in both cases assuming no jitter).”
Spectroscopic parameters for 451 stars in the HARPS GTO planet search program - Stellar [Fe/H] and the frequency of exo-Neptunes (2008, background): “…orbiting a solar-like star (Mayor & Queloz 1995), including several planets in the Neptune-mass regime (e.g. McArthur et al. 2004; Santos et al. 2004b; Butler et al. 2004; Vogt et al. 2005; Rivera et al. 2005; Bonfils et al. 2005a, 2007; Udry et al. 2006, 2007; Lovis et al. 2006; Melo et al. 2007).”
Tidal Evolution of Close-in Extrasolar Planets (2007, unknown): “…2007; Gillon et al. 2007; Johnson et al. 2006; Knutson et al. 2007; Laughlin et al. 2005; Lovis et al. 2006; McArthur et al. 2004; Maness 2007; Mayor 2004; Moutou et al. 2006; Rivera et al. 2005; Udry et al. 2002; Valenti & Fischer 2005; Vogt et al. 2005; Wright et al. 2006; and Zucker et al. 2004.”
Debris Disks around Sun-like Stars (2007, background): “…luminosity of 2:6 ; 10 5 based on 70 m photometry (the same data that are presented here). k This star has two known planets orbiting at 1.10 and 1.76 AU (Vogt et al. 2005). l Beichman et al. (2006a) derive a fractional luminosity of 0:7 ; 10 5 based on 70 m photometry and IRS spectroscopy.”
Improving the Efficiency of Markov Chain Monte Carlo for Analyzing the Orbits of Extrasolar Planets (2005, background): “HD 37124 Radial velocity observations of the star HD 37124 have revealed three planets (Vogt et al. 2005).”
TEN NEW AND UPDATED MULTIPLANET SYSTEMS AND A SURVEY OF EXOPLANETARY SYSTEMS (2008, background): “Vogt et al. (2005) updated the orbital fit, finding significant curvature in the residuals to the inner planet fit, and estimated its orbital period, though poorly constrained, to be 8.5 yr, with M sin i ∼ 2MJup.”
The Keck Planet Search: Detectability and the Minimum Mass and Orbital Period Distribution of Extrasolar Planets (2008, background): “For example, HD 128311 has two planets in a 2:1 resonance (Vogt et al. 2005).”
Catalog of Nearby Exoplanets (2006, background): “; K0: Korzennik et al. (2000); LC5: Lo Curto (2005); Le5: Lee et al. (2005); Lt9: Latham et al. (1989); Lv5: Lovis et al. (2005); MA4: McArthur et al. (2004); MC4: McCarthy et al. (2004), Mo5: Moutou et al. (2005); My3: http://obswww.unige.ch/∼naef/planet/geneva planets.html; My4: Mayor et al. (2004”
On the evolution of multiple protoplanets embedded in a protostellar disc (2006, background): “…and COROT will extend the discovery-space of extrasolar planets further, covering the sub-Neptune mass range where current observations typically cannot detect planets (e.g. Bonfils et al. 2005; Marcy et al. 2005; Rivera et al. 2005; Vogt et al. 2005; Santos et al. 2004; Butler et al. 2003, 2004).”